The accretion disks are known to be crucial structures which exist both in stellar scale in the vicinity of individual stars, and especially, in centers of galaxies, essentially determining the observational properties of those objects [1]}, [2]}, [3]}, [4]}, [5]}. Among the effects influencing the structure and evolution of accretion disks, General Relativity (GR) predictions i.e. Lense-Thirring, Bardeen-Petterson effects [6]} have been considered both for stellar and galactic nuclei scale accretion processes, see [7]} and references therein.
